High‐frequency type II radio emissions associated with shocks driven by coronal mass ejections
- 1 August 1999
- journal article
- Published by American Geophysical Union (AGU) in Journal of Geophysical Research
- Vol. 104 (A8) , 16979-16991
- https://doi.org/10.1029/1999ja900143
Abstract
No abstract availableKeywords
This publication has 19 references indexed in Scilit:
- Comment on “Origin of coronal and interplanetary shocks: A new look with Wind spacecraft data” by N. Gopalswamy et al.Journal of Geophysical Research, 1999
- On the origin of solar metric type II burstsSolar Physics, 1999
- Origin of coronal and interplanetary shocks: A new look with Wind spacecraft dataJournal of Geophysical Research, 1998
- WIND/WAVES observations of man‐made radio transmissionsGeophysical Research Letters, 1996
- The Large-Scale Density Structure of the Solar Corona and the Heliospheric Current SheetThe Astrophysical Journal, 1996
- WAVES: The radio and plasma wave investigation on the wind spacecraftSpace Science Reviews, 1995
- Speeds of coronal mass ejections: SMM observations from 1980 and 1984‐1989Journal of Geophysical Research, 1994
- Energetic interplanetary shocks, radio emission, and coronal mass ejectionsJournal of Geophysical Research, 1987
- Solar radio burst and in situ determination of interplanetary electron densitySolar Physics, 1984
- A coronal transient associated with a high-speed type II burstThe Astrophysical Journal, 1983